Viewing archive of Tuesday, 26 February 2008

Solar activity report

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Report of Solar-Geophysical Activity 2008 Feb 26 2203 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 057 Issued at 2200Z on 26 Feb 2008

IA. Analysis of Solar Active Regions and Activity from 25-2100Z to 26-2100Z

Solar activity was very low. The only region on the visible disk is Region 983 (S06W54).
IB. Solar Activity Forecast
Solar activity is expected to be very low.
IIA. Geophysical Activity Summary 25-2100Z to 26-2100Z
The geomagnetic field was quiet. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels again today.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be quiet to unsettled on day one (27 February). Unsettled to active conditions are expected on days two and three (28 - 29 February) with isolated minor storm levels possible at high latitudes. The increase in activity is due to a recurrent coronal hole high speed wind stream.
III. Event Probabilities 27 Feb to 29 Feb
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       26 Feb 071
  Predicted   27 Feb-29 Feb  070/070/070
  90 Day Mean        26 Feb 075
V. Geomagnetic A Indices
  Observed Afr/Ap 25 Feb  001/003
  Estimated     Afr/Ap 26 Feb  003/005
  Predicted    Afr/Ap 27 Feb-29 Feb  007/008-010/015-012/015
VI. Geomagnetic Activity Probabilities 27 Feb to 29 Feb
A. Middle Latitudes
Active15%20%25%
Minor storm05%05%05%
Major-severe storm01%01%01%
B. High Latitudes
Active20%30%30%
Minor storm05%10%10%
Major-severe storm01%05%05%

All times in UTC

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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Iqaluit, NU
Nuuk
Reykjavik
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Monday, 24 March 2025
Coronal hole faces Earth

The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity. 

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13:55 UTC - Coronal hole

A transequatorial coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days

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02:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC

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